A spectacular new image captured by the Hubble Space Telescope shows bright-blue wisps of glowing gas and hot, sparkling, young stars within a satellite dwarf galaxy known as the Large Magellanic Cloud (LMC).

The LMC is one of the smaller satellite galaxies that orbit the Milky Way, and it's among a collection of galaxies known as the local group. It is one of the closest galaxies to Earth, at about 163,000 light-years away.

"These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs and filaments from the surrounding material," Hubble researchers said in a statement when debuting the photo.

Within this stellar nursery lies a butterfly-shaped cosmic cloud known as the Papillon Nebula. The region consists of vast amounts of dense gas that give way to the birth of new stars.

N159 is located south of the Tarantula Nebula, which is designated heic1402 - another region known for massive star birth within the LMC. The Tarantula Nebula is located 170,000 light-years from Earth and is believed to house hundreds of thousands of stars. Inside the Tarantula Nebula lies an incredibly bright region known as 30 Doradus, which is considered a hotspot for star formation, according to the statement, released jointly by NASA and the European Space Agency.

This beautiful new image, one of many taken by the Hubble telescope, was captured using Hubble's Advanced Camera for Surveys.

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